Are Post-Newtonian templates faithful and effectual in detecting gravitational signals from neutron star binaries?

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

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14 pages, 3 figures, accepted for publication in Phys. Rev. D

Scientific paper

10.1103/PhysRevD.66.064013

We compute the overlap function between Post-Newtonian (PN) templates and gravitational signals emitted by binary systems composed of one neutron star and one point mass, obtained by a perturbative approach. The calculations are performed for different stellar models and for different detectors, to estimate how effectual and faithful the PN templates are, and to establish whether effects related to the internal structure of neutron stars may possibly be extracted by the matched filtering technique.

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